DARWIN: towards the ultimate dark matter detector
2016
DARk matter
WImpsearch with liquid
xenoN(
DARWIN) will be an experiment for the direct detection of dark matter using a multi-ton liquid
xenon
time projection chamberat its core. Its primary goal will be to explore the experimentally accessible parameter space for
Weakly Interacting Massive Particles(
WIMPs) in a wide mass-range, until neutrino interactions with the target become an irreducible background. The prompt scintillation light and the charge signals induced by particle interactions in the
xenonwill be observed by VUV sensitive, ultra-low background photosensors. Besides its excellent sensitivity to
WIMPsabove a mass of 5 GeV/c2, such a detector with its large mass, low-energy threshold and ultra-low background level will also be sensitive to other rare interactions. It will search for solar
axions, galactic
axion-like particles and the neutrinoless
double-beta decayof 136-Xe, as well as measure the low-energy
solar neutrinoflux with <1% precision, observe coherent neutrino-nucleus interactions, and detect galactic supernovae. We present the concept of the
DARWINdetector and discuss its physics reach, the main sources of backgrounds and the ongoing detector design and R&D efforts.
Keywords:
-
Correction
-
Source
-
Cite
-
Save
224
References
409
Citations
NaN
KQI